Fermat’s and energy variation principles in field theory
In general relativity the light is assumed to propagate in the vacuum along null geodesic in a pseudo-Riemannian manifold. Besides the geodesics principle in a classical field theory there exists the Fermat's principle for stationary gravity fields.[1]
Fermat's principle
In more general case for conformally stationary spacetime [2] with coordinates a Fermat metric takes form
,
where conformal factor depending on time and space coordinates does not affect the lightlike geodesics apart from their parametrization.
Fermat's principle for a pseudo-Riemannian manifold states that the light ray path between points and corresponds to zero variation of action
,
where is any parameter ranging over an interval and varying along curve with fixed endpoints and .
Principle of stationary integral of energy
In principle of stationary integral of energy for a light-like particle's motion, the pseudo-Riemannian metric with coefficients is defined by a transformation
With time coordinate and space coordinates with indexes k,q=1,2,3 the line element is written in form
where is some quantity, which is assumed equal 1 and regarded as the energy of the light-like particle with . Solving this equation for under condition gives two solutions
where are elements of the four-velocity. Even if one solution, in accordance with making definitions, is .
With and even if for one k the energy takes form
In both cases for the free moving particle the lagrangian is
Its partial derivatives give the canonical momenta
and the forces
Momenta satisfy energy condition [3] for closed system
Standard variational procedure is applied to action
which is integral of energy. Stationary action is conditional upon zero variational derivatives δS/δxλ and leads to Euler–Lagrange equations
which is rewritten in form
After substitution of canonical momentum and forces they give motion equations of lightlike particle in a free space
and
Static spacetime
For the static spacetime the first equation of motion with appropriate parameter gives . Canonical momentum and forces will be
.
For the isotropic paths a transformation to metric is equivalent to replacement of parameter on . The curve of motion of lightlike particle in four-dimensional spacetime and value of energy are invariant under this reparametrization. Canonical momentum and forces take form
Substitution of them in Euler–Lagrange equations gives
.
This expression after some calculation becomes null geodesic equations
where are the second kind Christoffel symbols with respect to the given metric tensor.
So in case of the static spacetime the geodesic principle and the energy variational method as well as Fermat's principle give the same solution for the light propagation.
See also
References
- ↑ Landau, Lev D.; Lifshitz, Evgeny F. (1980), The Classical Theory of Fields (4th ed.), London: Butterworth-Heinemann, p. 273, ISBN 9780750627689
- ↑ Perlik, Volker (2004), "Gravitational Lensing from a Spacetime Perspective", Living Rev. Relativity, 7 (9), Chapter 4.2
- ↑ Landau, Lev D.; Lifshitz, Evgeny F. (1976), Mechanics Vol. 1 (3rd ed.), London: Butterworth-Heinemann, p. 14, ISBN 9780750628969